Astronomy: The Science of the Heavenly BodiesTodd, David P. (David Peck)
History
Astronomy: The Science of the Heavenly Bodies
Todd, David P. (David Peck)
Astronomy
So Newton conceived the idea of a mountain observatory, on the summit of
which, as he thought, the air would be not only cloudless, but so steady
and equable that the rays of light from the heavenly bodies might reach
the eye undisturbed by atmospheric tremors and quiverings which are
almost always present in the lower strata of the great ocean of air that
surrounds our planet.
This is the way Newton puts the question in his treatise on
_Opticks_--he says: "The Air through which we look upon the Stars, is in
a perpetual Tremor; as may be seen by the tremulous Motion of Shadows
cast from high Towers, and by the twinkling of the fix'd stars.... The
only remedy is a most serene and quiet Air, such as may perhaps be found
on the tops of the highest Mountains above the grosser Clouds."
Newton's suggestion is that the _highest_ mountains may afford the best
conditions for tranquillity; and it is an interesting coincidence that
the summits of the highest mountains, about 30,000 feet in elevation,
are at about the same level where the turbulence of the atmosphere most
likely ceases, according to the indications of recent meteorological
research. These heights are far above any elevations permanently
occupied as yet, but a good beginning has been made and results of great
value have already been reached.
Curiously, investigation of mountain peaks and their suitability for
this purpose was not undertaken till nearly two centuries after Newton,
when Piazzi Smyth in 1856 organized his expedition to the summit of a
mountain of quite moderate elevation, and published his "Teneriffe: an
Astronomer's Experiment." Teneriffe is an accessible peak of about
10,000 feet, on an island of the Canaries off the African coast, where
Smyth fancied that conditions of equability would exist; and on reaching
the summit with his apparatus and spending a few days and nights there,
he was not disappointed. Could he have reached an elevation of 13,000
feet, he would have had fully one-third of all the atmosphere in weight
below him, and that the most turbulent portion of all. Nevertheless, the
gain in steadiness of the atmosphere, providing "better seeing," as the
astronomer's expression is, even at 10,000 feet, was most encouraging,
and led to attempts on other peaks by other astronomers, a few of whom
we shall mention.
Davidson, an observer of the United States Coast Survey, with a broad
experience of many years in mountain observing, investigated the summit
of the Sierra Nevada mountains as early as 1872, at an elevation of
7,200 feet. His especial object was to make an accurate comparison
between elevated stations at different heights. He found the seeing
excellent, especially on the sun; but the excessive snowfall at his
station, 45 feet annually, was a condition very adverse to permanent
occupation.
Public-domain text, read in full here on John Shaqi.
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